Results of the MCMC fit of the SPHERE, NaCo, and NICI combined astrometric data of PDS 70 b reported in terms of statistical distribution matrix of the orbital elements a, e, i, Ω, ω, and tp. We restrained the PDS70 b solution set given by the MCMC to solutions with orbital plane making a tilt angle of less than 5° with respect to the disk midplane described by Keppler et al. (2018), i.e., i = 180°−49.8° and PA = 158.6°.
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